5XMM J031817.4-025809
5XMM-DR15 stacked source · SRCID 3005602220100009
Position:
03h18m17.42s -02d58m09.1s
(49.57260°, -2.96920°)
EP flux
3.02e-14
± 5.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.947)
Detections
1
| SRCID | 3005602220100009 |
|---|---|
| IAUNAME | 5XMM J031817.4-025809 |
| SC_RA | 03h18m17.42s (49.57260°) |
| SC_DEC | -02d58m09.1s (-2.96920°) |
| RADEC_ERR | 0.60 arcsec |
| LII / BII | 184.8191° / -47.4012° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52503.423 (2002-08-17 10:08:51.000 UTC) |
| MJD_LAST | 52503.706 (2002-08-17 16:56:53.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.02e-14 ± 5.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.41
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
-0.04
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.51
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.63
± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.561
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
Optical Monitor (OM)
- OM Source ID
- 928476
- Match probability
- 0.97
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.155 | 0.215 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.15e-14 (+2.6e-14 / −1.8e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.11e+21 (+1.5e+21 / −4.6e+20) cm−2 |
| Photon index (Γ) | 2.69 (+2.92 / −2.30) |
| DoF | 405 |
| p-value | 0.835 |
| Inter-instrument norm. | 1.02 (0.84–1.26) |
| Quality flag | 0 |
No variability data available for this source.
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.